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Prediction for CME (2014-09-09T00:16:00-CME-001)CME Observed Time: 2014-09-09T00:16ZiSWAS Layout URL: https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/6596/-1 CME Note: Associated with M4.6 flare (2014-09-08T23:12Z). CME Shock Arrival Time: 2014-09-11T22:56Z Observed Geomagnetic Storm Parameters due to CME: Max Kp: 5.0 Dst min. in nT: -31 Dst min. time: 2014-09-13T03:00Z Predicted Arrival Time: 2014-09-11T23:00Z Predicted geomagnetic storm max Kp range due to CME: 6.0 - 6.0 Prediction Method: WSA-ENLIL + Cone (NOAA/SWPC) Prediction Method Note: (Arrival Prediction by NOAA/SWPC submitted to this system by M. Leila Mays) (Submitted CME shock arrival time taken from the excerpted Forecast Discussion below and http://www.swpc.noaa.gov/wsa-enlil/). (Submitted Kp estimate is from the excerpted Forecast Discussion and 3-Day Forecast below). -- Product: Forecast Discussion Issued: 2014 Sep 10 0030 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center Solar Activity .24 hr Summary... Solar activity was at moderate levels due to the long-duration M4/1n flare at 09/0029 UTC from Region 2158 (N15E14, Dkc/beta-gamma-delta). This M4/1n flare had associated Type II (999 km/s estimated shock velocity) and Type IV radio sweeps, a 10cm (370 sfu) radio burst, and an asymmetrical, full-halo coronal mass ejection (CME) which was first observed in LASCO/C2 imagery at 09/0006 UTC. As previously reported, the majority of the ejecta appeared to be heading north and east of the Sun/Earth line, however, after detailed analysis forecasters have determined this event to contain an Earth-directed component. A NOAA Scale G2 (Moderate) Geomagnetic Storm Watch has been issued for 12 September with an estimated shock arrival time early in the day. Residual CME effects warrant a NOAA Scale G1 (Minor) Geomagnetic Storm Watch for 13 September. Regions 2158 and 2157 (S14E03, Ekc/beta-gamma-delta) continue to be the regions of interest as they are the largest and most magnetically complex on the visible solar disk. Region 2158 continued to consolidate in the spots just south of the large leader. Region 2157 was responsible for a C3/1n flare at 09/1226 UTC and showed signs of growth in its intermediate spots. There were no additional CMEs observed in satellite imagery during the reporting period. .Forecast... Solar activity is expected to be moderate (R1-R2/Minor-Moderate)with a chance for X-class flares (R3 or greater) for the next three days (10-12 Sep). Regions 2157 and 2158 continue to be the likely source of significant flare activity. Energetic Particles .24 hr Summary... The greater than 2 MeV electron flux at geosynchronous orbit was at normal levels. The greater than 10 MeV proton flux at geosynchronous orbit was still slightly elevated but continued a steady decline. The greater than 10 MeV proton flux reached a high of 3.8 pfu at 09/0110 UTC. .Forecast... The greater than 2 MeV electron flux is expected to be at normal to moderate levels with a chance for high levels over the next three days (10-12 Sep). A chance for an S1 (Minor) solar radiation storm remains for the next three days (10-12 Sep) due to the increasingly favorable locations of Regions 2157 and 2158. Solar Wind .24 hr Summary... Solar wind parameters at ACE were indicative of a nominal solar wind regime. Solar wind speeds began the period near 450 km/s and reported period-ending speeds in the 375 km/s range. IMF total field values remained steady between 2 nT to 5 nT throughout the period, while Bz fluctuated between +/-4 nT. Phi angle remained in a negative (toward) orientation for the majority of the period with slight variability into away (positive) solar sector orientation after 09/1600 UTC. .Forecast... Solar wind parameters are expected to become slightly enhanced on day one (10 Sep) as coronal hole high speed stream (CH HSS) influence begins. A solar sector boundary change from a negative (towards) to a positive (away) solar sector is necessary before observing impacts from this feature. Day two (11 Sep), conditions should return to near background levels as CH HSS effects subside. Day three (12 Sep), should see the arrival of the 09 Sep CME, early in the day, when an enhancement in the interplanetary magnetic field and a simultaneous increase in density, speed, and temperature are expected at the ACE spacecraft in conjunction with the forecasted shock arrival. Geospace .24 hr Summary... The geomagnetic field was quiet with two isolated periods of unsettled conditions between 09/0000-0300 UTC as well as 09/2100-09/2400 UTC. .Forecast... The geomagnetic field is expected to be at quiet to unsettled levels on day one (10 Sep) due to weak, positive-polarity CH HSS influence. A return to mostly quiet conditions is anticipated for day two (11 Sep) as CH HSS effects wane. Early on day three (12 Sep), the 09 Sep CME mentioned above is expected to impact the Earth's magnetosphere. Quiet to major storm (G2/Moderate) conditions are expected as a result. Thank you for using the Product Subscription Service. If you would like to remove a product subscription or update the personal information in your account, go to the Product Subscription Site. Please do not use the from address for correspondence, as it is not monitored. For comments or help, please contact SWPC Help. Product: 3-Day Forecast Issued: 2014 Sep 10 0030 UTC Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center A. NOAA Geomagnetic Activity Observation and Forecast The greatest observed 3 hr Kp over the past 24 hours was 3 (below NOAA Scale levels). The greatest expected 3 hr Kp for Sep 10-Sep 12 2014 is 6 (NOAA Scale G2). NOAA Kp index breakdown Sep 10-Sep 12 2014 Sep 10 Sep 11 Sep 12 00-03UT 2 2 2 03-06UT 3 1 4 06-09UT 2 1 6 (G2) 09-12UT 2 1 5 (G1) 12-15UT 2 1 4 15-18UT 1 1 4 18-21UT 2 2 3 21-00UT 3 2 4 Rationale: No G1 (Minor) or greater geomagnetic storms are expected on days one and two (10-11 Sep). G1-G2 (Minor-Moderate) geomagnetic storms are expected on day three (12 Sep) due to effects from the 09 Sep CME. B. NOAA Solar Radiation Activity Observation and Forecast Solar radiation, as observed by NOAA GOES-13 over the past 24 hours, was below S-scale storm level thresholds. Solar Radiation Storm Forecast for Sep 10-Sep 12 2014 Sep 10 Sep 11 Sep 12 S1 or greater 30% 30% 30% Rationale: A chance for S1 (Minor) solar radiation storms exists due to potential flare activity from Regions 2157 (S14E03) and 2158 (N15E14) as well as already enhanced background conditions. C. NOAA Radio Blackout Activity and Forecast Radio blackouts reaching the R1 levels were observed over the past 24 hours. The largest was at Sep 09 2014 0030 UTC Radio Blackout Forecast for Sep 10-Sep 12 2014 Sep 10 Sep 11 Sep 12 R1-R2 75% 75% 75% R3 or greater 30% 30% 30% Rationale: R1-R2 (Minor-Moderate) radio blackouts are expected with a chance for R3 (Strong) activity due to flare potential from Regions 2157 and 2158. Thank you for using the Product Subscription Service. If you would like to remove a product subscription or update the personal information in your account, go to the Product Subscription Site. Please do not use the from address for correspondence, as it is not monitored. For comments or help, please contact SWPC Help.Lead Time: 53.55 hour(s) Difference: -0.07 hour(s) Prediction submitted by Leila Mays (GSFC) on 2014-09-09T17:23Z |
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